Zobrazeno 1 - 10
of 1 103
pro vyhledávání: '"Liu Wei-Min"'
Publikováno v:
E3S Web of Conferences, Vol 145, p 02070 (2020)
Guangdong-Hong Kong-Macao Greater Bay Area (GBA) is highly developed, characterized by obvious geographical advantages, excellent natural resources, continuous improvement of environmental quality, and accumulation of scientific and technological inn
Externí odkaz:
https://doaj.org/article/111bb920010a4a2bb0d20ffef9b44846
Publikováno v:
MNRAS 523, 907 (2023)
The disc instability mechanism (DIM) is widely accepted to account for the transient behaviour of dwarf novae (DNe), which experience short outbursts separated by long quiescence. The duty cycle (the ratio between the outburst duration and the recurr
Externí odkaz:
http://arxiv.org/abs/2308.08298
Publikováno v:
A&A 668, A80 (2022)
Ultracompact cataclysmic variables (CVs) of the AM CVn type are deemed to be important verification sources for the future space gravitational wave detectors such as the Laser Interferometer Space Antenna (LISA). We model the present-day Galactic pop
Externí odkaz:
http://arxiv.org/abs/2210.08434
Autor:
Zhang, Yi-Wang, Zhao, Chang, Su, Bo-Jing, Lin, Wei-Zheng, Liu, Wei-Min, Liang, Jing, Shao, Chun-Kui, Cheng, Na, Chen, Jian-Ning
Publikováno v:
In Annals of Diagnostic Pathology December 2024 73
Publikováno v:
In Ocean Engineering 1 December 2024 313 Part 3
Publikováno v:
In Ocean Engineering 15 June 2024 302
Autor:
Jiang, L., Wang, Na, Chen, Wen-Cong, Liu, Wei-Min, Leng, Chun-wei, Yuan, Jian-Ping, Qian, Xiang-Li
PSR J$1946+3417$ is a millisecond pulsar (MSP) with a spin period $P\simeq3.17\rm~ms$. Harbored in a binary with an orbital period $P_{\rm b}\simeq27$ days, the MSP is accompanied by a white dwarf (WD). The masses of the MSP and the WD were determine
Externí odkaz:
http://arxiv.org/abs/2106.05717
The space gravitational wave (GW) detector Laser Interferometer Space Antenna (LISA) that was planed to launch in the early 2030s is to detect the low-frequency GW signals in the Galaxy. AM CVn stars were generally thought to be important low-frequen
Externí odkaz:
http://arxiv.org/abs/2101.09850
Publikováno v:
In Ocean Engineering 15 February 2024 294
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